The Gaia-ESO survey: dynamical models of flattened, rotating globular clusters

We present a family of self-consistent axisymmetric rotating globular cluster models which are fitted to spectroscopic data for NGC 362, NGC 1851, NGC 2808, NGC 4372, NGC 5927 and NGC 6752 to provide constraints on their physical and kinematic properties, including their rotation signals. They are c...

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Bibliographic Details
Main Author: Jeffreson, Sarah (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: 2017
In: Arxiv

Online Access:Verlag, kostenfrei, Volltext: http://arxiv.org/abs/1704.07833
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Author Notes:Sarah M.R. Jeffreson, Jason L. Sanders, N.W. Evans, Angus A. Williams, G. F. Gilmore, Amelia Bayo, Angela Bragaglia, Ettore Flaccomio, Richard Jackson, Robert D. Jeffries, Paul Jofre, Carmela Lardo, Lorenzo Morbidelli, Elena Pancino, Simone Zaggia
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